Showing 1–20 of 31 results
/ Date/ Name
Nov 10, 2022The Star Formation Rate of the Milky Way as seen by HerschelMar 1, 2024Orbital analysis of stars in the nuclear stellar disc of the Milky WayMay 8, 2018First metallicity determination from Near-Infrared spectra for five obscured Cepheids discovered in the inner DiskJun 24, 2021The filamentary structures in the CO emission toward the Milky Way diskJun 17, 2021Dense molecular gas properties on 100 pc scales across the disc of NGC 3627Feb 10, 2017Kink Instability of Force-Free Jets: a Parameter Space StudyApr 30, 2017A Common Central Engine for Long Gamma Ray Bursts and Type Ib/c Supernovae?Sep 23, 2024Metallicity-dependent kinematics and orbits in the Milky Way's nuclear stellar discDec 10, 2025Rhea-RT: Dynamical impact of Central Molecular Zone conditions on ISM properties and stellar feedback couplingJan 22, 2019On the ridges, undulations & streams in Gaia DR2: Linking the topography of phase-space to the orbital structure of an N-body barSep 23, 2022ALMA uncovers highly filamentary structure towards the Sgr E regionSep 13, 2023Smooth kinematic and metallicity gradients reveal that the Milky Way's nuclear star cluster and disc might be part of the same structureMay 11, 2022Linking stellar populations to HII regions across nearby galaxies: I. Constraining pre-supernova feedback from young clusters in NGC1672Feb 6, 2023Evidence of an age gradient along the line of sight in the nuclear stellar disc of the Milky WayMay 26, 2023The Gas Morphology of Nearby Star-Forming GalaxiesMar 19, 2024Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamicsJul 19, 2024Star Formation in Extreme Environments: A 200 pc High Velocity Gas Stream in the Galactic CentreDec 9, 2025Chemical analysis of the Milky Way's Nuclear Star Cluster: Evidence for a metallicity gradientDec 13, 2022Synthetic dust polarization emission maps at 353 GHz for an observer placed inside a Local Bubble-like cavityJan 10, 2023Study of the excess Fe XXV line emission in the central degrees of the Galactic centre using XMM-Newton data